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In this paper, we report the relative SNe contributions on the metal budgetof the ICM of Abell 1837 galaxy cluster at redshift z $=$ 0.069. For thispurpose, we analysed the hot ICM of the cluster and obtained radial metaldistributions by using XMM-Newton archival data with total exposure $\sim$100ks. These metal measurements consist of Mg, Si, S, Fe and Ni within 0.7R$_{500}$ radius which is divided into three concentric annuli. In order toexplain the observed metal abundance pattern in terms of relative supernovacontributions, we used our newly developed code SNeRatio which utilizestheoretical nucleosynthesis models. This study covers the most recent 3D SNIaand SNcc yield tables. All combinations of these theoretical yields were fittedwith our measured abundance ratios and statistically acceptable ones wereselected. Each of these models were found to predict a uniform SNIa percentagecontribution to the total SNe from the cluster center to the outskirts and forman SNIa ratio distribution with a mean 39 $\pm$ 14$\%$. This uniformity isconsistent with the early enrichment scenario which assumes that the metalproduction processes begin in early phase of cluster formation, namelyproto-cluster phase at epoch z $\geq$ 2.

The Relative Supernovae Contribution to the Chemical Enrichment History of Abell 1837